The origin of the low-fluence component in the solar system.

Computer Science

Scientific paper

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Stellar Interiors: Nucleosynthesis, Massive Stars: Nucleosynthesis

Scientific paper

It is shown that the bulk of the solar system low-fluence s-process
component can be explained as resulting mainly from the neutron capture
nucleo-synthesis in central He-burning in massive stars. The
contribution of massive stars to the bulk solar abundance of
180Ta is also discussed.

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